Abstract
We derive new identities for the thermodynamic variables of five-dimensional,
asymptotically flat, stationary and biaxisymmetric vacuum black holes. These
identities depend on the topology of the solution and include contributions arising from certain topological charges. The proof employs the harmonic map formulation of the vacuum Einstein equations for solutions with these symmetries.
asymptotically flat, stationary and biaxisymmetric vacuum black holes. These
identities depend on the topology of the solution and include contributions arising from certain topological charges. The proof employs the harmonic map formulation of the vacuum Einstein equations for solutions with these symmetries.
| Original language | English |
|---|---|
| Number of pages | 10 |
| Journal | Classical and quantum gravity |
| Volume | 36 |
| Issue number | 07LT02 (9pp) |
| Early online date | 22 Feb 2019 |
| DOIs | |
| Publication status | Published - 12 Mar 2019 |
Keywords / Materials (for Non-textual outputs)
- general relativity in higher dimensions, black hole
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James Lucietti
- School of Mathematics - Personal Chair of Mathematical Physics
Person: Academic: Research Active